赤偏移2.6の銀河の塵からの偏熱放射
J E Geach1, E Lopez-Rodriguez2, M J Doherty3
1Centre for Astrophysics Research, School of Physics, Engineering and Computer Science, University of Hertfordshire, Hatfield, UK. j.geach@herts.ac.uk.
Nature
|September 6, 2023
まとめ
初期の銀河は 恒星形成に不可欠な 秩序ある磁場を形成しました 観測により 遠い銀河の磁場が5キロパルセックで 宇宙の歴史の中で これらの構造が急速に発展していることが明らかになった.
科学分野:
- 天体物理学
- 宇宙の進化
- 銀河の力学
背景:
- 磁場は銀河の進化,星間媒介,星形成に不可欠です.
- 大規模な磁場は近くの銀河で知られていますが 初期の宇宙の形成は不明です
研究 の 目的:
- 初期の宇宙における磁場の形成と構造を調査する.
- 銀河の磁場が 素早く形成されているか調べる
主な方法:
- 塵粒からの線形偏熱放射の検出
- レッドシフト2.6で強いレンズで輝く銀河の観測.
- 地元の磁場との塵粒の配列の分析
主要な成果:
- 5キロパルセックスケールの 磁場が検出されました
- 磁場強度は約500μG以下と推定される.
- 近隣の渦巻き銀河と似ています.
- 磁場は分子ガスの円盤に平行して方向づけられている.
結論:
- オーダーされた磁場は 銀河で急速に形成されます
- これらの構造は 宇宙の歴史の初期に存在していました
- 発見は 初期の銀河の進化と星形成における 磁場の役割を支持しています
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